Tracers confirm downward mixing of Tyrrhenian Sea upper waters associated with the Eastern Mediterranean Transient

14Citations
Citations of this article
24Readers
Mendeley users who have this article in their library.

Abstract

Observations of tritium and 3He in the Tyrrhenian Sea, 1987-2009, confirm the enhanced vertical mixing of intermediate waters into the deep waters that has been noted and associated with the Eastern Mediterranean Transient in previous studies. Our evidence for the mixing rests on increasing tracer concentrations in the Tyrrhenian deep waters, accompanied by decreases in the upper waters, which are supplied from the Eastern Mediterranean. The downward transfer is particularly evident between 1987 and 1997. Later on, information partly rests on increasing tritium-3He ages; here we correct the observed 3He for contributions released from the ocean floor. The Tyrrhenian tracer distributions are fully compatible with data upstream of the Sicily Strait and in the Western Mediterranean. The tracer data show that mixing reached to the bottom and confirm a cyclonic nature of the deep water circulation in the Tyrrhenian. They furthermore indicate that horizontal homogenization of the deep waters occurs on a time scale of roughly 5 years. Various features point to a reduced impact of Western Mediterranean Deep Water (WMDW) in the Tyrrhenian during the enhanced-mixing period. This is an important finding because it implies less upward mixing of WMDW, which has been named a major process to enable the WMDW to leave the Mediterranean via the Gibraltar Strait. On the other hand, the TDW outflow for several years represented a major influx of enhanced salinity and density waters into the deep-water range of the Western Mediterranean. © 2011 Author(s).

Figures

  • Fig. 1. Map of stations used in the present work. Station numbers are given next to the markings. For cruises see Table 1. Depth isolines are 500 m apart. Malta Escarpment = steep slope near 1995 Sta. 8; Sardinian Channel = deep connection between Tyrrhenian and WMed south of Sardinia.
  • Table 1. The cruises providing data.
  • Fig. 2. δ3He versus depth in 1987 (METEOR cruise 5/6), 1997 (POSEIDON cruise 234) and 2007/2009 (AEOLIAN 07 and ETYMED). For cruises see Table 1 and for station positions see Fig. 1. δ3He is defined as the relative deviation (%) from the atmospheric 3He/4He ratio. Due to different solubility of the two isotopes (cf. Sect. 1), δ3He has surface values near −1.6%.
  • Fig. 3. Density (σ2 = potential density anomaly referenced to 2000 dbar) versus salinity for Tyrrhenian stations, 1987–2007 and for WMed stations of 1997 (bottle data; the 1997 profiles are in color). For cruises and station positions see Table 1 and Fig. 1, depth markings are in dbar. For the 2007 tracer station a nearby CTD profile is shown (MEDOCC07, see Table 1), which displays staircase structures.
  • Fig. 5. Tritium, tritiugenic 3He [TU] and tritium-3He age [years/10] in the Tyrrhenian Sea in 1987 (M 5/6, Sta. 786, full lines), 1997 (POSEIDON 234, Sta. 766, dotted) and 2007 (AEOLIAN 07, V07B01, dashed). For station positions see Fig. 1. The scatter in the 1987 tritium profile and in the age profiles reflects the data uncertainties (Sect. 3).
  • Fig. 4. Profiles of tritium and tritiugenic 3He (both in TU) and of tritium-3He ages (Stas. 764 and 766 only) in the Tyrrhenian Sea and the WMed, POSEIDON 234, 1997. Note that age scale is compressed 10-fold (1 unit = 10 years). For station positions see Fig. 1. Sta. 736 in the WMed replaces 738 shown in Fig. 3 which does not have tracer data, while T and S are nearly the same. Tritium data for station 766 converted from Sta. 765 data using a correlation with the tracer CFC-12 (Sect. 3).
  • Fig. 6. Profiles of tritium, tritiugenic 3He [TU] and tritium-3Heages [years/5], Meteor 5/6, 1987, in the Tyrrhenian Sea (Sta. 786) and at the Malta Escarpment upstream of the Sicily Strait (Sta. 779). For Sta. 779 only the upper 1000 m are shown, for station positions see Fig. 1.
  • Fig. 7. Profiles of tritium and tritiugenic 3He off the Malta Escarpment in 1987 (METEOR 5/6, Sta. 779), 1995 (METEOR 31/1, Sta. 8), 1999 (METEOR 44/4, Sta. 303) and 2001 (METEOR 51/2, Sta. 558). For station positions see Fig. 1. The locations of the 1999 and 2001 stations are somewhat farther away from the escarpment. Note temporal inversions in the general trend of decreasing tracer concentrations.

References Powered by Scopus

Circulation in the Western Mediterranean Sea

1073Citations
N/AReaders
Get full text

Determination of tritium by mass spectrometric measurement of <sup>3</sup>He

488Citations
N/AReaders
Get full text

Comprehensive Review and Critical Evaluation of the Half-Life of Tritium

435Citations
N/AReaders
Get full text

Cited by Powered by Scopus

Physical forcing and physical/biochemical variability of the Mediterranean Sea: A review of unresolved issues and directions for future research

160Citations
N/AReaders
Get full text

The Mediterranean Sea system: A review and an introduction to the special issue

147Citations
N/AReaders
Get full text

Acidification of the Mediterranean Sea from anthropogenic carbon penetration

55Citations
N/AReaders
Get full text

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Cite

CITATION STYLE

APA

Roether, W., & Lupton, J. E. (2011). Tracers confirm downward mixing of Tyrrhenian Sea upper waters associated with the Eastern Mediterranean Transient. Ocean Science, 7(1), 91–99. https://doi.org/10.5194/os-7-91-2011

Readers over time

‘12‘13‘14‘15‘16‘17‘18‘19‘21‘2302468

Readers' Seniority

Tooltip

Researcher 11

52%

PhD / Post grad / Masters / Doc 10

48%

Readers' Discipline

Tooltip

Earth and Planetary Sciences 9

47%

Environmental Science 7

37%

Chemistry 2

11%

Physics and Astronomy 1

5%

Save time finding and organizing research with Mendeley

Sign up for free
0